Useful Information
USEFUL INFORMATION Radiation and Radioactivity Radioactivity is a characteristic of some elements that have unstable atomic nuclei, which spontaneously disintegrate or “decay” into atomic nuclei of another isotope or element. The nuclei decay until only a stable, nonradioactive isotope remains. Depending on the isotope, this process can take anywhere from less than a second to billions of years. Atoms that emit radiation are called radionuclides. Radionuclides are unstable isotopes of an element that have the same number of protons but different numbers of neutrons, resulting in different atomic masses. For example, the element hydrogen has two stable isotopes, hydrogen•1 ( 1H) and hydrogen•2 ( 2H) (deuterium), and one radioactive isotope, hydrogen•3 (3H) (tritium). The superscript preceding the element’s symbol identifies the atomic mass, which is the number of protons plus neutrons in the nucleus. Thus, 1H has one proton and no neutrons, 2H has one proton and one neutron, and3H has one proton and two neutrons. When radioactive atoms decay by emitting radiation, the daughter products that result may be either radioactive or stable. Generally, radionuclides with high atomic numbers, such as uranium•238 and plutonium•239, have many generations of radioactive progeny. For example, the radioactive decay of plutonium•239 creates uranium•235, thorium•231, protactinium•231, and so on, through 11 progeny until only the stable isotope lead•207 remains. Radionuclides with lower atomic numbers often have no more than one daughter. For example, strontium•90 has one radioactive daughter, yttrium•90, which finally decays into stable zirconium; cobalt•60 decays directly to stable nickel with no intermediate nuclide.
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